3D structure of the Milky Way out to 10 kpc from the Sun - Catalogue of large molecular clouds in the Galactic Plane

Open Access

Fig. 7

Comparison between our clouds and molecular clouds observed in CO. Left panel: 3D distribution of molecular clouds observed in CO from Miville-Deschênes et al. (2017), with our extracted clouds over-plotted as contours. Right panel: longitude-velocity plot of molecular clouds from the left, situated underneath our cloud contours. The colour shows the surface density of clouds derived in Miville-Deschênes et al. (2017).

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